Every point of a wavefront (or of an aperture lit by a wave) acts as a secondary source emitting a spherical wavelet, in phase with the wave there; the wave beyond is the coherent sum of the wavelets. For an aperture lit by a plane wave of amplitude , the amplitude reaching a far point is , with the phase of the path from the aperture point to ( a constant). Fraunhofer (far-field) diffraction is the case where is at infinity — or in the focal plane of a lens — so that the rays from all points of the aperture toward are parallel, in the direction , and
The pattern is observed at infinity, or at the focus of a lens, where the direction of small angles maps to the point .
Examples
Example 22.5 (Eye, telescope, microscope)
The eye (, ): , about — a detail at , which is indeed about the acuity of a good eye: evolution matched the retina’s cells to the diffraction limit. A telescope: , a thousand times better, if the atmosphere lets it (it does not, from the ground: of "seeing", whence space telescopes and adaptive optics). A radio dish of at : , worse than the eye; interferometers across continents restore the resolution. A microscope objective of aperture angle resolves — about in the visible, whatever the magnification: the limit that drove microscopy to electrons and to X-rays.